Photometric solution of the eclipsing binary system EF Bootis

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dc.contributor.authorÖzdemir, S
dc.contributor.authorDemircan, O
dc.contributor.authorÇiçek, C
dc.contributor.authorErdem, A
dc.date.accessioned2025-01-27T21:00:01Z
dc.date.available2025-01-27T21:00:01Z
dc.date.issued2004
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractThe EF Boo eclipsing binary system is studied in the context of optical light curves and radial velocity curves published in the literature. The best-solution leads to an over-contact configuration of W-subclass of W UMa systems with a fill-out factor of 28%. Absolute parameters based on simultaneous solution of light and radial velocity curves are presented.
dc.identifier.doi10.1002/asna.200310174
dc.identifier.endpage335
dc.identifier.issn0004-6337
dc.identifier.issue4
dc.identifier.scopus2-s2.0-4644337099
dc.identifier.scopusqualityQ3
dc.identifier.startpage332
dc.identifier.urihttps://doi.org/10.1002/asna.200310174
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26914
dc.identifier.volume325
dc.identifier.wosWOS:000221547300007
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWiley-V C H Verlag Gmbh
dc.relation.ispartofAstronomische Nachrichten
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectbinaries : eclipsing
dc.subjectbinaries : close
dc.subjectstars : individual (EF Bootis)
dc.titlePhotometric solution of the eclipsing binary system EF Bootis
dc.typeArticle

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